Abstract
Details are presented of the Whipple Observatory's 10 m atmospheric Cherenkov telescope and camera, as it evolved during the period 1997 until 2006. The design of the telescope and camera's optical and electronic systems is discussed together with a detailed description of the four-stage GRANITE (Gamma-RAy New Imaging TElescope) upgrade program, undertaken during the same time period. The objective of the upgrade was to improve the telescope's sensitivity for the detection of very-high-energy gamma-rays. Results from the program are provided and are briefly discussed in the context of the design of VERITAS.
Original language | English (US) |
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Pages (from-to) | 182-195 |
Number of pages | 14 |
Journal | Astroparticle Physics |
Volume | 28 |
Issue number | 2 |
DOIs | |
State | Published - Oct 2007 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics